Peculiar behavior of ion-electron plasma and pair plasma in blackhole magnetospheres
Project/Area Number |
21540243
|
Research Category |
Grant-in-Aid for Scientific Research (C)
|
Allocation Type | Single-year Grants |
Section | 一般 |
Research Field |
Astronomy
|
Research Institution | Kumamoto University |
Principal Investigator |
KOIDE Shinji 熊本大学, 大学院・自然科学研究科, 教授 (20234677)
|
Project Period (FY) |
2009 – 2012
|
Project Status |
Completed (Fiscal Year 2012)
|
Budget Amount *help |
¥3,510,000 (Direct Cost: ¥2,700,000、Indirect Cost: ¥810,000)
Fiscal Year 2012: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2011: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2010: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2009: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
|
Keywords | ブラックホール磁気圏 / 通常プラズマ / 対プラズマ / 一般化 GRMHD 方程式 / ブラックホール / GRMHD方程式 / プラズマ / ホール効果 / 熱起電力 / 電気抵抗 / 磁気リコネクション / カーブラックホール / 一般相対論的電磁流体力学 / エルゴ領域 |
Research Abstract |
We have investigated the peculiar effects of ion-electron (normal)plasma and positron-electron (pair) plasma using generalized general relativistic MHD(GRMHD) equations. It showed clearly that the peculiar effects are limited to Hall andthermo-electromotive force effects. First, it shows Hall effect may become significantfor normal plasmas of gamma-ray bursts and microquasars, however it disappears for pairplasmas. The term of thermo-electromotive force may becomes larger than the classicalresistivity for both normal and pair plasmas of gamma-ray bursts, micro-quasars, andactive galactic nuclei, however, it is not expected to become significant because it willnot cause drastic phenomena like magnetic reconnection, which is caused with resistivity
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Report
(5 results)
Research Products
(36 results)